Equation of state in neutron stars and supernovae
arXiv:2207.00033 · doi:10.1007/978-981-15-8818-1_104-1
Abstract
Neutron stars and supernovae provide cosmic laboratories of highly compressed matter at supra nuclear saturation density which is beyond the reach of terrestrial experiments. The properties of dense matter is extracted by combining the knowledge of nuclear experiments and astrophysical observations via theoretical frameworks. A matter in neutron stars is neutron rich, and may further accommodate non-nucleonic degrees of freedom such as hyperons and quarks. The structure and composition of neutron stars are determined by equations of state of matter, which are the primary subject in this chapter. In case of supernovae, the time evolution includes several dynamical stages whose descriptions require equations of state at finite temperature and various lepton fractions. Equations of state also play essential roles in neutron star mergers which allow us to explore new conditions of matter not achievable in static neutron stars and supernovae. Several types of hadron-to-quark transitions, from first order transitions to crossover, are reviewed, and their characteristics are summarized.
arXiv comment53 pages, 24 figures, Contribution to the "Handbook of Nuclear Physics", Springer, 2022, edited by I. Tanihata, H. Toki and T. Kajino
References in corpus (131)
- Shapiro delay measurement of a two solar mass neutron star
- A Massive Pulsar in a Compact Relativistic Binary
- The equation of state for nucleon matter and neutron star structure
- GW170817: Measurements of Neutron Star Radii and Equation of State
- How Massive Single Stars End their Life
- The order of the quantum chromodynamics transition predicted by the standard model of particle physics
- PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
- Neutron Star Structure and the Equation of State
- QCD Phenomenology based on a Chiral Effective Lagrangian
- Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar
- Color superconductivity in dense quark matter
- Construction of high-quality Nucleon-Nucleon potential models
- Masses, Radii, and Equation of State of Neutron Stars
- Explosion Mechanisms of Core-Collapse Supernovae
- Color-Flavor Locking and Chiral Symmetry Breaking in High Density QCD
- Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event
- A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
- Equations of state for supernovae and compact stars
- Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral
- Gravitational-wave constraints on the neutron-star-matter Equation of State
- Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620
- The Nuclear Equation of State and Neutron Star Masses
- Composition and thermodynamics of nuclear matter with light clusters
- Neutron Star Cooling
- Constraints on a phenomenologically parameterized neutron-star equation of state
- Quantum Monte Carlo methods for nuclear physics
- Constraining the Maximum Mass of Neutron Stars From Multi-Messenger Observations of GW170817
- Using gravitational-wave observations and quasi-universal relations to constrain the maximum mass of neutron stars
- From hadrons to quarks in neutron stars: a review
- Black Hole Formation in Failing Core-Collapse Supernovae
- Phases of Dense Quarks at Large N_c
- Core-collapse supernova equations of state based on neutron star observations
- Constraints on the symmetry energy and neutron skins from experiments and theory
- Hybrid stars that masquerade as neutron stars
- Physics of Neutron Star Crusts
- New constraints on radii and tidal deformabilities of neutron stars from GW170817
- Skyrme Interaction and Nuclear Matter Constraints
- Statistical Model for a Complete Supernova Equation of State
- Binary and Millisecond Pulsars
- Evolution of Protoneutron Stars
- Minimal Cooling of Neutron Stars: A New Paradigm
- Neutron-star radius constraints from GW170817 and future detections
- Binary neutron-star mergers: a review of Einstein's richest laboratory
- Superconductivity by long-range color magnetic interaction in high-density quark matter
- Constraining the Symmetry Parameters of the Nuclear Interaction
- Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview
- GW170817, General Relativistic Magnetohydrodynamic Simulations, and the Neutron Star Maximum Mass
- Measuring the neutron star equation of state using X-ray timing
- Perspectives on Core-Collapse Supernova Theory
- The Cooling of Compact Stars
- Identifying a first-order phase transition in neutron star mergers through gravitational waves
- Signatures of quark-hadron phase transitions in general-relativistic neutron-star mergers
- Chiral interactions up to next-to-next-to-next-to-leading order and nuclear saturation
- On the Mass Distribution and Birth Masses of Neutron Stars
- Quarkyonic Matter and Neutron Stars
- Supernova Neutrino Detection
- Constraining the Equation of State of Neutron Stars from Binary Mergers
- Maximum mass, moment of inertia and compactness of relativistic stars
- The Neutron Star Mass Distribution
- Explosion Mechanism, Neutrino Burst, and Gravitational Wave in Core-Collapse Supernovae
- Constraint on the maximum mass of neutron stars using GW170817 event
- The search for failed supernovae with the Large Binocular Telescope: confirmation of a disappearing star
- The Minimal CFL-Nuclear Interface
- Neutron stars - cooling and transport
- A way forward in the study of the symmetry energy: experiment, theory, and observation
- Neutron Stars and the Nuclear Equation of State
- A Survey About Nothing: Monitoring a Million Supergiants for Failed Supernovae
- The Compression-Mode Giant Resonances and Nuclear Incompressibility
- Merger and Mass Ejection of Neutron-Star Binaries
- The Diffuse Supernova Neutrino Background is detectable in Super-Kamiokande
- Strangeness in Nuclei and Neutron Stars
- Multimessenger Parameter Estimation of GW170817
- Incompressibility in finite nuclei and nuclear matter
- Hadron-Quark Crossover and Massive Hybrid Stars with Strangeness
- Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
- Nucleon Effective Masses in Neutron-Rich Matter
- Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae
- Nuclear equation of state for core-collapse supernova simulations with realistic nuclear forces
- New Neutron Star Equation of State with Quark-Hadron Crossover
- Detection of Neutrinos from Supernovae in Nearby Galaxies
- Chiral Effective Field Theory and the High-Density Nuclear Equation of State
- Gravitational waves from newly born, hot neutron stars
- Phenomenological QCD equation of state for massive neutron stars
- Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase
- Hadron-quark mixed phase in hyperon stars
- and N interactions from Lattice QCD near the physical point
- Hadron-Quark Crossover and Massive Hybrid Stars
- dibaryon from lattice QCD near the physical point
- Perturbative Thermal QCD: Formalism and Applications
- Soft interactions in cold quark matter
- Properties of Neutrino-driven Ejecta from the Remnant of Binary Neutron Star Merger : Purely Radiation Hydrodynamics Case
- A long-lived remnant neutron star after GW170817 inferred from its associated kilonova
- Equation of state of nuclear and neutron matter at third-order in perturbation theory from chiral EFT
- Neutrino flavour transformation in supernovae
- Astrophysical Implications of Equation of State for Hadron-Quark Mixed Phase: Compact Stars and Stellar Collapses
- Neutrino signals from the formation of black hole: a probe of equation of state of dense matter
- Neutrino-driven Explosions
- Dynamical Derivation of the Momentum Space Shell Structure for Quarkyonic Matter
- Laboratory Tests of Low Density Astrophysical Equations of State
- Constraining the onset density of the hadron-quark phase transition with gravitational-wave observations
- Cold quark matter at N3LO: soft contributions
- Effects of symmetry energy on equation of state for simulations of core-collapse supernovae and neutron-star mergers
- Neutrino Emission from Supernovae
- Neutron stars with hyperon cores: stellar radii and EOS near nuclear density
- Gravitational wave asteroseismology with protoneutron stars
- Merger and post-merger of binary neutron stars with a quark-hadron crossover equation of state
- Hard-core deconfinement and soft-surface delocalization from nuclear to quark matter
- Implications of NICER for neutron star matter: the QHC21 equation of state
- Neutrino Emission as Diagnostics of Core-Collapse Supernovae
- A new equation of state for core-collapse supernovae based on realistic nuclear forces and including a full nuclear ensemble
- Variational study for the equation of state of asymmetric nuclear matter at finite temperatures
- Equation of state for neutron stars with hyperons by the variational method
- Possible early linear acceleration of proto-neutron stars via asymmetric neutrino emission in core-collapse supernovae
- Stiffening of matter in quark-hadron continuity
- Comparing treatments of weak reactions with nuclei in simulations of core-collapse supernovae
- Constraining supernova equations of state with equilibrium constants from heavy-ion collisions
- Influence of the symmetry energy on nuclear pasta in neutron star crusts
- Observing Supernova Neutrino Light Curves with Super-Kamiokande: Expected Event Number over 10 s
- Dense 2-color QCD towards continuum and chiral limits
- Properties of dense, asymmetric nuclear matter in Dirac-Brueckner-Hartree-Fock approach
- Two-colour QCD phases and the topology at low temperature and high density
- Dependence of weak interaction rates on the nuclear composition during stellar core collapse
- Hadron-quark mixed phase in the quark-meson coupling model
- Probing Rotation of Core-collapse Supernova with Concurrent Analysis of Gravitational Waves and Neutrinos
- The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
- Can chiral EFT give us satisfaction?
- Influence of density dependence of symmetry energy in hot and dense matter for supernova simulations
- Reexamining the relation between the binding energy of finite nuclei and the equation of state of infinite nuclear matter
- Properties of neutrino transfer in a deformed remnant of neutron star merger
- Nuclei in Core-Collapse Supernovae Engine
- Numerical Study of Stellar Core Collapse and Neutrino Emission Using the Nuclear Equation of State Obtained by the Variational Method